Speaker
Isaac Vidaña
(INFN Sezione di Catania )
Description
In this part we will analyze the importance of the nuclear EoS on the properties of neutron stars. We will discuss the main open challenges in the description of the EoS, mainly focussing on the limits of the current many-body techniques, the so-called "hyperon puzzle" and the dependence of cooling properties on the nuclar EoS.
